Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Innovative real-time processing for solar adaptive optics
    Themis is a 90 cm solar telescope which undergoes a rejuvenation of its scientific instruments. In particular, it is about to be equipped with an adaptive optics (AO) system with a bandwidth of at least 1 kHz and featuring a 97 actuator deformable mirror and 10×10 Shack-Hartmann wavefront sensor. Nowadays, the computational power required by such a
    Thiébaut, Éric et al.

    Advertised on:

    7
    2018
    Citations
    0
  • Innovative aspects to shrink the volume of the future laser guide star facility for the Gran Telescopio Canarias adaptive optics system
    This contribution is focused on the innovative aspects of the design of the Laser Guide Star (LGS) Facility for the Gran Telescopio Canarias (GTC) Adaptive Optics (GTCAO) System [6]. After a trade-off process considering different alternatives, a preliminary opto-mechanical design was defined, based on a "TOPTICA SodiumStar" laser to be launched on
    Sánchez Capuchino, J. et al.

    Advertised on:

    7
    2018
    Citations
    0
  • Impact of young stellar components on quiescent galaxies: deconstructing cosmic chronometers
    Context. Cosmic chronometers may be used to measure the age difference between passively evolving galaxy populations to calculate the Hubble parameter H(z) as a function of redshift z. The age estimator emerges from the relationship between the amplitude of the rest frame Balmer break at 4000 Å and the age of a galaxy, assuming that there is one
    López-Corredoira, M. et al.

    Advertised on:

    7
    2018
    Citations
    36
  • High-redshift BL Lac Objects: Spectroscopy of Candidates
    We report on 16 BL Lacertae objects that were proposed to be at z > 1. We present spectroscopic observations secured at the 10.4 m GTC that allowed us to assess the redshift of these sources. In particular, for five objects, we disprove the previous value of the redshift reported in the literature and found that they lie at z 1. Moreover, two of
    Landoni, M. et al.

    Advertised on:

    7
    2018
    Citations
    23
  • High redshift galaxies in the ALHAMBRA survey. II. Strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 ≤ z≤ 4.5 by PDF analysis
    Context. Knowing the exact shape of the ultraviolet (UV) luminosity function (LF) of high-redshift galaxies is important to understand the star formation history of the early Universe. However, the uncertainties, especially at the faint and bright ends of the LFs, remain significant. Aims: In this paper, we study the UV LF of redshift z = 2.5 - 4.5
    Viironen, K. et al.

    Advertised on:

    7
    2018
    Citations
    11
  • HARMONI pre-optics design at PDR
    HARMONI is a visible and near-infrared (0.5 to 2.45 μm) integral field spectrograph, providing the E-ELT's core spectroscopic capability, over a range of resolving powers from R (λ/Δλ) 3500 to 18000. The instrument provides simultaneous spectra of ˜32000 spaxels arranged in a sqrt(2):1 aspect ratio contiguous field. The pre-optics take light
    Cagigas, M. A. et al.

    Advertised on:

    7
    2018
    Citations
    0